Observation details report
Detailed source parameters (including errors) in a comma-separated values file
Click on source number for detailed analysis, including spectral fits if applicable
| data | idnum | idradec | telescope | instrument | x | y | cnts | cntserr | rate | rateerr | SNR | poisprob | sigmaj | sigmin | incang | offax | cnts_soft | cnts_hard | hr | hr_err | ext | var | N_H | flux | vign | flags | |
|---|---|---|---|---|---|---|---|---|---|---|---|---|---|---|---|---|---|---|---|---|---|---|---|---|---|---|---|
| Report | srcpi bgdpi arf rmf | 1 | X041937.93+022437.1 | chandra | ccd1 | 537.833 | 658.784 | 152.125 | 21.4564 | 0.0157699 | 0.00222425 | 12.2528 | 1 | 1.65265 | 1.65265 | 0 | 3.13868 | T | T | 1.02e+21 | 9.00732e-14 | 1 | dsxf | ||||
| Report | srcpi bgdpi arf | 6 | X041930.67+022236.8 | chandra | ccd1 | 758.826 | 414.156 | 57.5166 | 7.58657 | 0.0059624 | 0.000786454 | 4.63264 | 0.999994 | 0.709024 | 0.709024 | 0 | 3.77263 | F | F | 1.01e+21 | 6.68103e-14 | 1 | dsx | ||||
| Report | srcpi bgdpi arf | 1 | X042012.64+022859.8 | chandra | ccd3 | 401.109 | 686.239 | 44.6475 | 7.34855 | 0.0046298 | 0.000762021 | 11.6558 | 1 | 1.15254 | 0.841205 | 37.5266 | 9.62051 | F | T | 1.04e+21 | 6.08816e-14 | 1 | dx | ||||
| Report | srcpi bgdpi arf | 10 | X041959.10+023134.3 | chandra | ccd3 | 813.578 | 1000.21 | 43.2327 | 7.1415 | 0.00448309 | 0.000740551 | 11.2864 | 1 | 4.33712 | 2.09161 | 26.4132 | 10.0191 | A | F | 1.05e+21 | 5.98888e-14 | 1 | dx | ||||
| Report | srcpi bgdpi arf | 6 | X042010.61+021940.3 | chandra | ccd2 | 969.236 | 451.382 | 30.6762 | 6.52479 | 0.00318104 | 0.000676603 | 8.89382 | 1 | 1.26144 | 1.26144 | 0 | 6.70023 | F | F | 1.01e+21 | 3.70465e-14 | 1 | dsx | ||||
| Report | srcpi bgdpi arf | 9 | X042003.91+023157.1 | chandra | ccd3 | 667.072 | 1046.45 | 15.4782 | 4.58265 | 0.00160504 | 0.000475207 | 4.04077 | 0.999864 | 3.59539 | 2.57218 | 28.9854 | 10.8257 | F | F | 1.05e+21 | 2.20612e-14 | 1 | dx | ||||
| Report | srcpi bgdpi arf | 5 | X042000.28+023049.2 | chandra | ccd3 | 777.9 | 908.928 | 17.7183 | 5.69132 | 0.00183735 | 0.000590179 | 4.62557 | 0.999974 | 4.69252 | 1.63232 | 141.184 | 9.44005 | A | F | 1.04e+21 | 2.40785e-14 | 1 | dsx | ||||
| Report | srcpi bgdpi arf | 4 | X042015.81+021752.6 | chandra | ccd2 | 810.389 | 232.056 | 15.0819 | 4.24268 | 0.00156395 | 0.000439953 | 4.37263 | 0.999884 | 2.36449 | 1.44266 | 78.4367 | 8.65148 | A | F | 1.01e+21 | 1.92523e-14 | 1 | dx | ||||
| Report | srcpi bgdpi arf | 5 | X042011.85+022023.3 | chandra | ccd2 | 931.033 | 538.433 | 13.4096 | 3.87301 | 0.00139054 | 0.000401619 | 3.8878 | 0.999729 | 1.977 | 0.953174 | 61.8322 | 6.77151 | A | F | 1.01e+21 | 1.62425e-14 | 1 | dx | ||||
| Report | srcpi bgdpi arf | 8 | X042014.61+023147.4 | chandra | ccd3 | 340.921 | 1026.87 | 12.4526 | 4.35903 | 0.0012913 | 0.000452017 | 3.2509 | 0.998743 | 5.39844 | 3.499 | 175.906 | 12.0666 | A | F | 1.05e+21 | 1.85564e-14 | 1 | dx | ||||
| Report | srcpi bgdpi arf | 2 | X042008.70+022526.4 | chandra | ccd3 | 521 | 252.5 | 11.972 | 3.74169 | 0.00124146 | 0.000388002 | 3.12543 | 0.997522 | 0.58344 | 0.5535 | 90 | 6.63955 | F | F | 1.03e+21 | 1.49338e-14 | 1 | dx | ||||
| Report | srcpi bgdpi arf | 4 | X041952.38+023025.3 | chandra | ccd3 | 1018.25 | 859.833 | 8.82274 | 3.46416 | 0.000914891 | 0.000359223 | 2.30328 | 0.984516 | 2.10176 | 1.40353 | 114.34 | 8.45717 | F | F | 1.04e+21 | 1.16088e-14 | 1 | dx | ||||
| Report | srcpi bgdpi arf | 1 | X041955.61+021605.1 | chandra | ccd0 | 485.75 | 469.5 | 7.58152 | 2.82843 | 0.000786181 | 0.0002933 | 2.57613 | 0.992138 | 0.932617 | 0.787075 | 126.091 | 6.53878 | F | T | 9.96e+20 | 9.33363e-15 | 1 | dx | ||||
| Report | srcpi bgdpi arf | 6 | X042014.45+022656.9 | chandra | ccd3 | 345.9 | 436.3 | 7.28308 | 3.16233 | 0.000755232 | 0.000327924 | 1.90133 | 0.956038 | 1.93944 | 1.21127 | 29.8914 | 8.65566 | A | F | 1.03e+21 | 9.66092e-15 | 1 | dx | ||||
| Report | srcpi bgdpi arf | 2 | X041942.57+021358.6 | chandra | ccd0 | 882.929 | 212.357 | 6.51157 | 2.64576 | 0.000675231 | 0.000274358 | 2.21257 | 0.983838 | 0.758525 | 0.492 | 112.5 | 8.19236 | A | F | 9.86e+20 | 8.50204e-15 | 1 | dx | ||||
| Report | srcpi bgdpi arf | 3 | X041948.94+021629.6 | chandra | ccd0 | 688.773 | 519.318 | 10.7389 | 3.31663 | 0.00111359 | 0.000343925 | 3.64898 | 0.999329 | 0.836431 | 0.492 | 115.705 | 5.69857 | A | F | 9.95e+20 | 1.29049e-14 | 1 | dx | ||||
| Report | srcpi bgdpi arf | 4 | X041943.88+021650.5 | chandra | ccd0 | 843.447 | 562.225 | 25.7019 | 5.0697 | 0.00266524 | 0.000525718 | 8.73328 | 1 | 1.29232 | 1.29232 | 0 | 5.29234 | F | F | 9.95e+20 | 3.06044e-14 | 1 | dsx | ||||
| Report | srcpi bgdpi arf | 5 | X041939.23+021900.7 | chandra | ccd0 | 984.611 | 826.5 | 8.48326 | 3.00001 | 0.00087969 | 0.000311092 | 2.88254 | 0.996367 | 0.661105 | 0.492 | 2.40726e-08 | 3.50826 | F | F | 1e+21 | 9.79078e-15 | 1 | dx | ||||
| Report | srcpi bgdpi arf | 7 | X042007.66+021552.9 | chandra | ccd0 | 118.5 | 444.667 | 9.46656 | 3.46415 | 0.000981654 | 0.000359222 | 3.21665 | 0.998402 | 2.46086 | 1.31311 | 77.4447 | 8.32501 | A | F | 9.99e+20 | 1.21898e-14 | 1 | dx | ||||
| Report | srcpi bgdpi arf | 8 | X042004.82+021614.5 | chandra | ccd0 | 205.214 | 488.643 | 6.15845 | 2.64577 | 0.000638613 | 0.000274359 | 2.09259 | 0.968504 | 1.86217 | 0.986326 | 138.262 | 7.5904 | A | F | 9.99e+20 | 7.76367e-15 | 1 | dx | ||||
| Report | srcpi bgdpi arf | 9 | X041948.92+021552.4 | chandra | ccd0 | 689.964 | 444.149 | 34.4213 | 7.1933 | 0.00356941 | 0.00074593 | 11.6961 | 1 | 0.856489 | 0.856489 | 0 | 6.30656 | F | F | 9.93e+20 | 4.20881e-14 | 1 | dsx |
counts and rate are bgd.-subtracted, based on simple spatial fitting (if done) or extracted counts from aperture otherwise (N.B., in either case aperture counts are given csv file).
cntserr, rateerr = Error on (source) counts and count rate, based on error in total counts
SNR = signal-to-noise ratio, computed using Nsrc/sqrt(Nbgd)
poisprob = Poisson probability of observing total counts given bgd. counts
sigmaj, sigmin = source extent (from detection output or spatial fitting) in units of arcsecs.
incang = position angle of source (inclination from x-axis)
cnts_soft = bgd.-subtracted counts in soft band (0.50 - 2.00 KeV, always taken directly from source aperture rather than model fitting)
cnts_hard = bgd.-subtracted counts in hard band (2.00 - 7.99 KeV, always taken directly from source aperture rather than model fitting)
hr, hr_err = hardness ratio ([cnts_hard-cnts_soft]/[cnts_hard+cnts_soft]) and error
ext = source extension flag: F = false (not extended), T = true (extended), A = asymetric (ratio of sigmaj/sigmin > 1 + x, where x = 0.5 by default)
var = variability flag: U = unknown, F = false (is not variable), T = true
N_H = Galactic column density as determined from LHEASOFT nh program
flux = flux determined from count rate using pimms (in the 0.30-8.00 keV bandpass for a power-law model with ph. index = 1.8)
vign = vignetting correction
Flags: d = detection parameters, s = simple spatial fitting parameters,
b = simple spatial fitting failed, p = poor simple spatial fit, x = extracted events parameters, t = temporal anaylsis parameters,
i = psf spatial fitting parameters, f = spectral fitting parameters,
c = source is confused, u = user-defined source, v = detected source coincident with user-defined source, r = source is in region-of-interest